Observing the WHIM with Athena

T. Brand, J. Wilms, T. Dauser, P. Peille, B. Cobo, M. Ceballos, R. A. den Hartog, J. S. Kaastra, P. O'Brien, X. Barcons, L. Piro, J.-W. A. den Herder (+4 others)
2016 Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray  
We present simulations of the detection probability for absorption lines from ions in the warm and hot ionized medium (WHIM) with Athena in the spectra of Gamma-ray burst afterglows. The simulations are based on Swift XRT lightcurves of these afterglows and are performed using the end-to-end simulation framework SIXTE. We simulate both the case of single and multiple absorption lines, as well as results for line searches in absorption structures from a more complex medium. We show that the
more » ... a X-IFU can detect WHIM lines with strong Ovii lines (equivalent widths larger than 0.14 eV) in spectra containing 3 × 10 6 counts. Downloaded From: http://proceedings.spiedigitallibrary.org/ on 08/17/2016 Terms of Use: http://spiedigitallibrary.org/ss/termsofuse.aspx Proc. of SPIE Vol. 9905 99055F-2 Downloaded From: http://proceedings.spiedigitallibrary.org/ on 08/17/2016 Terms of Use: http://spiedigitallibrary.org/ss/termsofuse.aspx Proc. of SPIE Vol. 9905 99055F-7 Downloaded From: http://proceedings.spiedigitallibrary.org/ on 08/17/2016 Terms of Use: http://spiedigitallibrary.org/ss/termsofuse.aspx
doi:10.1117/12.2234442 fatcat:7xgl4kw365cqxnvsvwzbkddst4